High response photochromic films based on D-A diarylethenes and their application in holography.


Journal

RSC advances
ISSN: 2046-2069
Titre abrégé: RSC Adv
Pays: England
ID NLM: 101581657

Informations de publication

Date de publication:
09 Jul 2020
Historique:
received: 24 06 2020
accepted: 02 07 2020
entrez: 6 5 2022
pubmed: 13 7 2020
medline: 13 7 2020
Statut: epublish

Résumé

A set of photochromic dithienylethenes bearing amino and nitro groups are synthesised and embedded at high concentrations in a polymer matrix (Cellulose Acetate Butyrate, CAB) to produce films showing a large reversible modulation of the complex refractive index in the Vis-NIR spectral range, thanks to an interesting combination of remarkable response at the molecular level and very high load capability in the chosen matrix. The photochromic derivatives are characterized in solution and in CAB films by means of electronic and vibrational spectroscopy, complemented by DFT calculations. Both the real and imaginary part of the refractive index are determined by spectroscopic ellipsometry. The modulation of the refractive index in the near infrared is in the range 0.02-0.04. These are very large values for such kinds of systems and they are due to a favourable combination of very large solubility of the derivatives in CAB and a high polarisability change. As for the change in transparency in the visible, contrast values larger than 10

Identifiants

pubmed: 35519783
doi: 10.1039/d0ra05535b
pii: d0ra05535b
pmc: PMC9055363
doi:

Types de publication

Journal Article

Langues

eng

Pagination

26177-26187

Informations de copyright

This journal is © The Royal Society of Chemistry.

Déclaration de conflit d'intérêts

There are no conflicts to declare.

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Auteurs

Maria Chiara Mantero (MC)

INAF - Osservatorio Astronomico di Brera Via Bianchi 46 23807 Merate Italy andrea.bianco@inaf.it.

Luca Oggioni (L)

INAF - Osservatorio Astronomico di Brera Via Bianchi 46 23807 Merate Italy andrea.bianco@inaf.it.

Giorgio Pariani (G)

INAF - Osservatorio Astronomico di Brera Via Bianchi 46 23807 Merate Italy andrea.bianco@inaf.it.

Fausto Ortica (F)

Dipartimento di Chimica, Biologia e Biotecnologie, Università Degli Studi di Perugia Via Elce di Sotto 8 Perugia 06123 Italy.
Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Perugia Via Pascoli Perugia 06123 Italy.

Silvano Tosi (S)

Dipartimento di Fisica, Università di Genova Via Dodecaneso 33 Genova 16146 Italy.
INFN, Sezione di Genova Via Dodecaneso 33 Genova 16146 Italy.

Maurizio Canepa (M)

OPTMATLAB, Dipartimento di Fisica, Università di Genova Via Dodecaneso 33 Genova 16146 Italy.

Chiara Bertarelli (C)

Dipartimento di Chimica, Materiali e Ingegneria Chimica, Politecnico di Milano Piazza Leonardo da Vinci 32 20133 Milano Italy.
Center for Nano Science and Technology, Istituto Italiano di Tecnologia Via Pascoli 10 20133 Milano Italy.

Matteo Tommasini (M)

Dipartimento di Chimica, Materiali e Ingegneria Chimica, Politecnico di Milano Piazza Leonardo da Vinci 32 20133 Milano Italy.

Andrea Bianco (A)

INAF - Osservatorio Astronomico di Brera Via Bianchi 46 23807 Merate Italy andrea.bianco@inaf.it.

Classifications MeSH